80 China Gears up for Lunar Science
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Space-VLBI Observations 1
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Space-VLBI observations 1 1999 Mon. Not. R. Astron. Soc. 000, 1{7 (2000) Space-VLBI observations of OH maser OH34.26+0.15: low interstellar scattering V.I. Slysh,1 M.A. Voronkov,1 V. Migenes,2 K.M. Shibata,3 T. Umemoto,3 V.I. Altunin,4 I.E. 1Astro Space Centre of Lebedev Physical Institute, Profsoyuznaya 84/32, 117810 Moscow, Russia 2University of Guanajuato, Department of Astronomy, Apdo Postal 144, Guanajuato, CP36000, GTO, Mexico 3National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181, Japan 4Jet Propulsion Laboratory, 4800 Oak Grove Dr., Pasadena, CA 91109, USA 5National Radio Astronomy Observatory, 520 Edgemont Rd., Charlottesville, VA 22903, USA 6Special Research Bureau, Moscow Power Engineering Institute, Krasnokazarmennaya st. 14, 111250 Moscow, Russia 7Dominion Radio Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council, PO Box 248, Penticton, BC, Canada V2A 6K3 8Australia Telescope National Facility, PO Box 76, Epping, NSW 2121, Australia 9Shanghai Astronomical Observatory, 80 Nandan Rd, Shanghai 200080, China 10Institute of Applied Astronomy, Zhdanovskaya str. 8, 197042 St.Petersburg, Russia Received date; accepted date ABSTRACT We report on the first space-VLBI observations of the OH34.26+0.15 maser in two main line OH transitions at 1665 and 1667 MHz. The observations involved the space radiotelescope on board the Japanese satellite HALCA and an array of ground radio telescopes. The map of the maser region and images of individual maser spots were pro- duced with an angular resolution of 1 milliarcsec which is several times higher than the angular resolution available on the ground. -
Chang'e 5 Samples (Mexag) (Head-Final)
Chang’E 5 Lunar Sample Return Mission Update James w. Head Department of Earth, Environmental and Planetary Sciences Brown University Providence, RI 02912 USA Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting: April 7 - 8, 2021. Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting Barbara Cohen, ExMAG Chair. 2/10/21 • 1. Please provide an update on the Chang'e 5 Sample Return Mission. • 2. What is known of the collection so far? • 3. Please provide an overview of allocation procedures. • 4. Since US federally-funded researchers cannot work directly with China - Who outside of China is working with the mission team? • 5. We'd also appreciate your thoughts on: What NASA might be able to do to enable the US analysis community to collaborate on this sample collection? Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting Barbara Cohen, ExMAG Chair. 2/10/21 • 1. Some Myths and Realities. • 2. Organization of the Chinese Space Program. • 3. Chinese Lunar Exploration Program (CLEP) context for Chang’e 5. • 4. Chang’e 5 Landing Site Selection, Global Context, Key Questions, Mission Operations and Sample Return. • 5. Returned Sample Location, Storage, Preliminary Analysis and Distribution. • 6. Opportunities for International Cooperation. Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting Barbara Cohen, ExMAG Chair. 2/10/21 • 1. Some Myths and Realities. • 2. Organization of the Chinese Space Program. • 3. Chinese Lunar Exploration Program (CLEP) context for Chang’e 5. • 4. Chang’e 5 Landing Site Selection, Global Context, Key Questions, Mission Operations and Sample Return. • 5. Returned Sample Location, Storage, Preliminary Analysis and Distribution. • 6. Opportunities for International Cooperation. -
The VSOP Survey: Final Individual Results R
The VSOP Survey: Final individual results R. Dodson∗ a,† S. Horiuchib, W. Scottc, E. Fomalontd, Z. Paragie, S. Frey f , K. Wiikg, H. Hirabayashia, P. Edwardsh, Y. Murataa, G. Moellenbrockd, L. Gurvitse, and S. Tingayb aISAS, JAXA, 3-1-1 Yoshinodai, Sagamihara, Japan bCentre for Astrophysics and Supercomputing, University of Swinburne, Melbourne, Australia cPhysics and Astronomy Department, University of Calgary, Canada d National Radio Astronomy Observatory, Charlottesville, U.S. eJoint Institute for VLBI in Europe, Dwingeloo, Netherlands f FÖMI Satellite Geodetic Observatory, Budapest, Hungary gTuorla Observatory, Piikkiö, Finland hAustralia Telescope National Facility, CSIRO, Sydney, Australia E-mail: [email protected] In February 1997 the Japanese radio astronomy satellite HALCA was launched to provide the space-borneelement for the VSOP mission. HALCA providedlinear baselines three-times greater than that of ground arrays, thus providing higher resolution and higher AGN brightness temper- ature measurements and limits. Twenty-five percent of the scientific time of the mission was devoted to the “VSOP survey” of bright, compact, extra-galactic radio sources at 5 GHz. A complete list of 294 survey targets were selected from pre-launch surveys, 91% of which were observed during the satellite’s lifetime. The major goals of the VSOP Survey are statistical in nature: to determine the brightness temperature and approximate structure, to provide a source arXiv:astro-ph/0612373v2 20 Dec 2006 list for use with future space VLBI missions, and to compare radio properties with other data throughout the electromagnetic spectrum. All the data collected have now been analysed and is being prepared for the final image Survey paper. -
Ebook Download Quantum Enhancement of a 4 Km Laser Interferometer Gravitational-Wave Detector 1St Edition
QUANTUM ENHANCEMENT OF A 4 KM LASER INTERFEROMETER GRAVITATIONAL-WAVE DETECTOR 1ST EDITION PDF, EPUB, EBOOK Sheon S Y Chua | 9783319367026 | | | | | Quantum Enhancement of a 4 Km Laser Interferometer Gravitational-Wave Detector 1st edition PDF Book Imaging 10 2 Google Scholar. Chua, B. Skip to main content. After the split light repeatedly bounces back and forth within each arm, the two beams then pass back through the beam splitter into a photodetector. But either way, it breaks a record. Thankfully, these passing gravitational waves are imperceptible to our human bodies, but the detectors of LIGO and Virgo are sensitive enough to pick them up. Cosmic Vision. Further, it showed that the presence of a squeezed-light source added no additional noise in the low frequency band. Noll, D. Comparison between the observed laser beam frequency in return beam and the local laser beam frequency sent beam encodes the wave parameters. When a gravitational wave passes the interferometer, the lengths of the two LISA arms vary due to space-time distortions caused by the wave. Gravitational-wave astronomy. Applied Phys. Help Learn to edit Community portal Recent changes Upload file. Botter, S. Ward, Laser phase and frequency stabilization using an optical resonator. Principles of Digital and Analog Communications , 2nd edn. Khalaidovski, H. General relativity Tests of general relativity Metric theories Graviton. And if a gravitational wave passes through while the two light pulses are bouncing back and forth within each perpendicular arm, the space-time within the detector arms would be disproportionately distorted. Potential sources for signals are merging massive black holes at the centre of galaxies , [15] massive black holes [16] orbited by small compact objects , known as extreme mass ratio inspirals , binaries of compact stars in our Galaxy, [17] and possibly other sources of cosmological origin, such as the very early phase of the Big Bang , [18] and speculative astrophysical objects like cosmic strings and domain boundaries. -
Satellite Observations of Pulsating Stars
Satellite Observations of Pulsating Stars Joanna Molenda-Zakowicz_ 1 1. University of Wroc law, Astronomical Institute, Kopernika 11, 51{622 Wroc law, Poland Presented are the impact of satellite observations on asteroseismic investigation and the programmes of ground-based follow-up observations dedicated to different space missions. 1 Asteroseismology from Space The second half of the XXth century provided astronomers with an invaluable oppor- tunity to observe stars from space. Since the satellite observatories are located above the Earth's atmosphere, data obtained with them do not suffer from distorting effects of the atmosphere and their acquisition is not limited by the weather conditions or the day-and-night cycle (but see Gadimova & Haubold, 2014, who discuss how the space weather affects satellite observations). As a result, space telescopes can obtain long, uninterrupted time-series of observations of a selected target or perform contin- uous mapping of the entire sky. Another important advantage of space missions is an opportunity to observe stars in these parts of the electromagnetic spectrum which does not reach the Earth's surface such as γ-rays, X-rays, far ultraviolet, and large parts of the infrared spectrum. The list of space telescopes which improved our understanding of the properties of pulsating stars is long. Among the most important ones there are: the astro- metric space mission Hipparcos (Lacroute, 1981), the Hubble Space Telescope (HST, Bahcall, 1986), the Wide Field Infrared Explorer (WIRE, Hacking & Werner, 1995), the Microvariability and Oscillations of STars telescope (MOST, Walker et al., 2003; Matthews, 2003), the Kepler space telescope and its continuation the K2 mission (Koch et al., 2004; Gilliland et al., 2010; Howell et al., 2014), the COnvection RO- tation and planetary Transits space mission (CoRoT, Baglin et al., 2006), and the BRIght Target Explorer (BRITE-Constellation, Weiss et al., 2014). -
Espinsights the Global Space Activity Monitor
ESPInsights The Global Space Activity Monitor Issue 3 July–September 2019 CONTENTS FOCUS ..................................................................................................................... 1 A new European Commission DG for Defence Industry and Space .............................................. 1 SPACE POLICY AND PROGRAMMES .................................................................................... 2 EUROPE ................................................................................................................. 2 EEAS announces 3SOS initiative building on COPUOS sustainability guidelines ............................ 2 Europe is a step closer to Mars’ surface ......................................................................... 2 ESA lunar exploration project PROSPECT finds new contributor ............................................. 2 ESA announces new EO mission and Third Party Missions under evaluation ................................ 2 ESA advances space science and exploration projects ........................................................ 3 ESA performs collision-avoidance manoeuvre for the first time ............................................. 3 Galileo's milestones amidst continued development .......................................................... 3 France strengthens its posture on space defence strategy ................................................... 3 Germany reveals promising results of EDEN ISS project ....................................................... 4 ASI strengthens -
Chang'e Flying to the Moon
Issue 7 January 2013 All about the Chinese Space Programme GO TAIKONAUTS! Editor’s Note COVER STORY If you are a fan of the Chinese space pro- gramme, you must have heard about Brian Harvey, who is the first Western writer to publish a book on the Chinese space pro- gramme. We are very happy that Mr. Harvey contributed an article to Go Taikonauts! The article about Chinese ... page 2 Quarterly Report October - December 2012 Launch Events China made six space launches in the last three months of 2012, setting a new annual launch record of 19 and overtaking U.S. in number of suc- cessful annual space launches for the first time. In 2011, China also ... page 3 Deep Space Adventure of Chang’e 2 From A Backup Lunar Orbiter to An Asteroid Probe Observation Just before Chang’e 1 (CE-1)’s successful mission to the Moon was completed, Echo of the Curiosity in China China announced that they would send the second lunar probe Chang’e 2 (CE-2) The 6 August 2012 was a special day to an to the Moon in 2010. No one at that time could anticipate the surprises that CE-2 American-Chinese girl. She is Clara Ma, would bring a few years later since it was just a backup ... page 8 a 15-year-old middle school student from Lenexa, Kansas. She waited for this day for more than three years. In May 2009, History Ma won a NASA essay contest for naming the Mars Science Laboratory, the most Chang’e Flying to the Moon complicated machine .. -
Chang'e-1 Lunar Mission: an Overview and Primary Science Results
0254-6124/2010/30(5)-392–12 Chin. J. Space Sci. Ouyang Ziyuan, Li Chunlai, Zou Yongliao, Zhang Hongbo, Lu Chang, Liu Jianzhong, Liu Jianjun, Zuo Wei, Su Yan, Wen Weibin, Bian Wei, Zhao Baochang, Wang Jianyu, Yang Jianfeng, Chang Jin, Wang Huanyu, Zhang Xiaohui, Wang Shijin, Wang Min, Ren Xin, Mu Lingli, Kong Deqing, Wang Xiaoqian, Wang Fang, Geng Liang, Zhang Zhoubin, Zheng Lei, Zhu Xinying, Zheng Yongchun, Li Junduo, Zou Xiaoduan, Xu Chun, Shi Shuobiao, Gao Yifei, Gao Guannan. Chang’E-1 lunar mission: an overview and primary science results. Chinese Journal of Space Science, 2010, 30(5): 392-403 Chang’E-1 Lunar Mission: An Overview and Primary Science Results Ouyang Ziyuan1,2 Li Chunlai1 Zou Yongliao1 Zhang Hongbo1 Lu Chang1 Liu Jianzhong1 Liu Jianjun1 Zuo Wei1 Su Yan1 Wen Weibin1 Bian Wei1 Zhao Baochang3 Wang Jianyu4 Yang Jianfeng3 Chang Jin5 Wang Huanyu6 Zhang Xiaohui7 Wang Shijin7 Wang Min1 Ren Xin1 Mu Lingli1 Kong Deqing1 Wang Xiaoqian1 Wang Fang1 Geng Liang1 Zhang Zhoubin1 Zheng Lei1 Zhu Xinying1 Zheng Yongchun1 Li Junduo1 Zou Xiaoduan1 Xu Chun1 Shi Shuobiao1 Gao Yifei1 Gao Guannan1 1(National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012) 2(Institute of Geochemistry, Chinese Academy of Sciences) 3(Xi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences) 4(Shanghai Institute of Technical Physics, Chinese Academy of Sciences) 5(Purple Mountain Observatory, Chinese Academy of Sciences) 6(Institute of High Energy Physics, Chinese Academy of Sciences) 7(Center for Space Science and Applied Research, Chinese Academy of Sciences) Abstract Chang’E-1 is the first lunar mission in China, which was successfully launched on Oct. -
The Hipparcos and Tycho Catalogues
The Hipparcos and Tycho Catalogues SP±1200 June 1997 The Hipparcos and Tycho Catalogues Astrometric and Photometric Star Catalogues derived from the ESA Hipparcos Space Astrometry Mission A Collaboration Between the European Space Agency and the FAST, NDAC, TDAC and INCA Consortia and the Hipparcos Industrial Consortium led by Matra Marconi Space and Alenia Spazio European Space Agency Agence spatiale europeenne Cover illustration: an impression of selected stars in their true positions around the Sun, as determined by Hipparcos, and viewed from a distant vantage point. Inset: sky map of the number of observations made by Hipparcos, in ecliptic coordinates. Published by: ESA Publications Division, c/o ESTEC, Noordwijk, The Netherlands Scienti®c Coordination: M.A.C. Perryman, ESA Space Science Department and the Hipparcos Science Team Composition: Volume 1: M.A.C. Perryman Volume 2: K.S. O'Flaherty Volume 3: F. van Leeuwen, L. Lindegren & F. Mignard Volume 4: U. Bastian & E. Hùg Volumes 5±11: Hans Schrijver Volume 12: Michel Grenon Volume 13: Michel Grenon (charts) & Hans Schrijver (tables) Volumes 14±16: Roger W. Sinnott Volume 17: Hans Schrijver & W. O'Mullane Typeset using TEX (by D.E. Knuth) and dvips (by T. Rokicki) in Monotype Plantin (Adobe) and Frutiger (URW) Film Production: Volumes 1±4: ESA Publications Division, ESTEC, Noordwijk, The Netherlands Volumes 5±13: Imprimerie Louis-Jean, Gap, France Volumes 14±16: Sky Publishing Corporation, Cambridge, Massachusetts, USA ASCII CD-ROMs: Swets & Zeitlinger B.V., Lisse, The Netherlands Publications Management: B. Battrick & H. Wapstra Cover Design: C. Haakman 1997 European Space Agency ISSN 0379±6566 ISBN 92±9092±399-7 (Volumes 1±17) Price: 650 D¯ ($400) (17 volumes) 165 D¯ ($100) (Volumes 1 & 17 only) Volume 2 The Hipparcos Satellite Operations Compiled by: M.A.C. -
China Dream, Space Dream: China's Progress in Space Technologies and Implications for the United States
China Dream, Space Dream 中国梦,航天梦China’s Progress in Space Technologies and Implications for the United States A report prepared for the U.S.-China Economic and Security Review Commission Kevin Pollpeter Eric Anderson Jordan Wilson Fan Yang Acknowledgements: The authors would like to thank Dr. Patrick Besha and Dr. Scott Pace for reviewing a previous draft of this report. They would also like to thank Lynne Bush and Bret Silvis for their master editing skills. Of course, any errors or omissions are the fault of authors. Disclaimer: This research report was prepared at the request of the Commission to support its deliberations. Posting of the report to the Commission's website is intended to promote greater public understanding of the issues addressed by the Commission in its ongoing assessment of U.S.-China economic relations and their implications for U.S. security, as mandated by Public Law 106-398 and Public Law 108-7. However, it does not necessarily imply an endorsement by the Commission or any individual Commissioner of the views or conclusions expressed in this commissioned research report. CONTENTS Acronyms ......................................................................................................................................... i Executive Summary ....................................................................................................................... iii Introduction ................................................................................................................................... 1 -
China Readies to Launch First Moon Rover Mission 30 November 2013
China readies to launch first moon rover mission 30 November 2013 "Apart from launching astronauts into space, this is probably the most complex space mission attempted by China," Australian space analyst Morris Jones told AFP. "It will also make China only the third nation to soft- land a spacecraft on the moon." Beijing sees its military-run space programme as a marker of its rising global stature and growing technological might, as well as the ruling Communist Party's success in turning around the fortunes of the once poverty-stricken nation. China has previously sent two probes to orbit the This file photo shows a model of a lunar rover 'Jade moon, with controllers sending the first of them Rabbit', seen on display at the China International crashing into the lunar surface at the end of its Industry Fair in Shanghai, on November 5, 2013 mission. China will launch its first ever moon rover mission on Monday, state media said, as Beijing embarks on the latest stage in its ambitious space programme. A rocket carrying the vehicle, named "Jade Rabbit" in a nod to Chinese folklore, will blast off at 1:30 am local time (Sunday 1730 GMT). "The Chang'e 3 is set to be launched for its moon mission from the Xichang Satellite Launch Center on Dec. 2," state broadcaster CCTV said on its verified Twitter account on Saturday. This file photo shows a rocket being blasted off from the Official news agency Xinhua also confirmed the launch centre in Xichang, China's southwestern province launch date, citing officials at the satellite launch of Sichuan, on October 1, 2010 centre in Sichuan province. -
Statement of Dr. Namrata Goswami
Statement of Dr. Namrata Goswami Independent Senior Analyst and Author 2016-2017 Minerva Grantee Before the U.S.-China Economic and Security Review Commission Hearing on “China in Space: A Strategic Competition?” April 25, 2019 This statement is submitted to the U.S.-China Economic and Security Review Commission (Commission), based on my decades old research on China as a major power in international politics and specifically of studying China’s space program. My focus today is on China’s space program and its long-term ambitions and goals. I would like to thank the Commission for this opportunity to appear before it. The Commission posed a few broad questions to me. I aim to answer them in the following order: a) What are the current status and future goals of China’s space exploration programs, including asteroid mining, a lunar base, and on-site resource exploitation? How capable is China of achieving these goals? b) To what degree are China’s civilian space programs guided by dual-use aims rather than purely civilian scientific research purposes? Related to that: how does China’s international sharing of the outcomes of its space scientific research reflect the primary aims of these programs? c) What access agreement terms China is offering prospective partners for its planned space station, and how successful has China been in attracting partners? d) policy recommendations. Current Status of China’s Space Program. China’s capability to launch, establish presence and conduct deep space exploration and resource utilization has undergone significant shifts in the last few decades.1 In 2018, China achieved the world’s largest number of space launches (39), compared to the U.S.